Английская Википедия:Einstein–Rosen metric

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Версия от 13:43, 2 марта 2024; EducationBot (обсуждение | вклад) (Новая страница: «{{Английская Википедия/Панель перехода}} {{Short description|Exact gravitational-wave solution to Einstein's field equations}} The '''Einstein–Rosen metric''' is an exact solution of Einstein's field equation. It was derived by Albert Einstein and Nathan Rosen in 1937.<ref>{{cite journal |author=Einstein, Albert |author2=Rosen, Nathan |name-list-style=amp |date=1937 |title=On Gravitational waves |journal=Journal...»)
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Шаблон:Short description The Einstein–Rosen metric is an exact solution of Einstein's field equation. It was derived by Albert Einstein and Nathan Rosen in 1937.[1] It is the first exact solution of Einstein's equation that described the propagation of a gravitational wave.

This metric can be written in a form such that the Belinski–Zakharov transform applies, and thus has the form of a gravitational soliton.

In 1972 and 1973, J. R. Rao, A. R. Roy, and R. N. Tiwari published a class of exact solutions involving the Einstein-Rosen metric.[2][3]\[4]

In 2021 Robert F. Penna found an algebraic derivation of the Einstein-Rosen metric.[5]

In the history of science, one might consider as a footnote to the Einstein-Rosen metric that Einstein, for some time, believed that he had found a non-existence proof for gravitational waves.[6]

Notes

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Шаблон:Relativity-stub